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Showing 1 to 20 of 27 for “"M33"”.

  1. Improving the extragalactic distance scale using Cepheids in M33

    … The first study uses Cepheids in two areas of M33; a sample from the metal-rich central region is compared with the more metal-poor sample from the southern spiral arm. Period-luminosity relations in the reddening-free Wesenheit index Wvi are constructed for the two samples and the measured …

    liverpool-jm Repository record for Improving the extragalactic distance scale using Cepheids in M33 (opens in a new tab)

  2. THE CEPHEIDS OF M33: DISTANCE AND METALLICITY EFFECTS THROUGH SLOAN FILTERS

    … 1.3 million stars in the nearby spiral galaxy M33. Over 1500 Cepheids were identified and Leavitt Laws were empirically derived. The slopes were found to be consistent with semi-empirical determinations. By adopting the semi-empirical slopes, a mean distance modulus of 24.57 ± 0.06 mag to the …

    liverpool-jm Repository record for THE CEPHEIDS OF M33: DISTANCE AND METALLICITY EFFECTS THROUGH SLOAN FILTERS (opens in a new tab)

  3. Kinematics and metallicity of RGB stars in the triangulum (M33) galaxy

    cambridge

  4. Point Process Modelling of Objects in the Star Formation Complexes of the M33 Galaxy

    … objects in the star formation complexes of the M33 galaxy. The GPP models circumvent the limitations of the two-point correlation function employed in the current astronomy literature by naturally accounting for the inhomogeneous distribution of these objects. The spatial distribution of these …

    uwo Repository record for Point Process Modelling of Objects in the Star Formation Complexes of the M33 Galaxy (opens in a new tab)

  5. Accreting Compact Objects in Technicolor: Multiwavelength Characterization of High Mass X-ray Binaries in the Local Group

    … resolved recent star formation history (SFH) of M33. In M31, I used observations from the Hubble Space Telescope (HST), the Chandra X-ray Observatory, and the Nuclear Spectroscopic Telescope Array (NuSTAR) to characterize the population of HMXBs in that galaxy and measure the overall HMXB …

    washington Repository record for Accreting Compact Objects in Technicolor: Multiwavelength Characterization of High Mass X-ray Binaries in the Local Group (opens in a new tab)

  6. Stochastinė galaktikų diskų evoliucija. 2-D modeliai /

    … the simulation of star formation history in the M33 galaxy. Based on the detailed analysis of the M33 galaxy evolution, we showed that, in order to resolve the evolution parameter degeneracy problem, it is necessary to use 2-D capabilities of the model as well as synthetic colour-magnitude …

    vilnius Repository record for Stochastinė galaktikų diskų evoliucija. 2-D modeliai / (opens in a new tab)

  7. The accuracy of integrated star clusters parameters. The effects of stochasticity /

    … from literature. For 747 star clusters in the M33 galaxy, available optical data have been supplemented with our near-infrared data measured on 2MASS images, and their age, mass, and extinction have been derived. A typical disruption time of star clusters in the M33 galaxy is found to ~300 Myr, …

    vilnius Repository record for The accuracy of integrated star clusters parameters. The effects of stochasticity / (opens in a new tab)

  8. Integralinių žvaigždžių spiečių parametrų tikslumas. Stochastiniai efektai /

    … from literature. For 747 star clusters in the M33 galaxy, available optical data have been supplemented with our near-infrared data measured on 2MASS images, and their age, mass, and extinction have been derived. A typical disruption time of star clusters in the M33 galaxy is found to ~300 Myr, …

    vilnius Repository record for Integralinių žvaigždžių spiečių parametrų tikslumas. Stochastiniai efektai / (opens in a new tab)

  9. Neutral hydrogen observations of spiral and irregular galaxies

    … two nearby galaxies af late spiral type, namely M33 and NGC 2403. The severe warping of the HI layer in the outer parts of M33 was clearly seen, and the origin of this phenomenon is discussed. Sensitive low-resolution maps reveal only a very slight warp in NGC 2403, while maps at the full …

    cambridge Repository record for Neutral hydrogen observations of spiral and irregular galaxies (opens in a new tab)

  10. Engineering human single-chain T cell receptors

    … murine T cells. The high affinity scTv, called m33, that is specific for the pepMHC SIY/Kb was used to redirect T cells with similar antigen sensitivity to the full-length m33 TCR. An inherent problem with full-length TCR gene therapy is the generation of receptors of unknown specificity through …

    uiuc Repository record for Engineering human single-chain T cell receptors (opens in a new tab)

  11. Made-to-measure Modelling of Nuclear Star Clusters

    … star cluster residing in the pure spiral galaxy M33.

    cent-lancashire Repository record for Made-to-measure Modelling of Nuclear Star Clusters (opens in a new tab)

  12. Estabilidad aerobica del ensilaje de marango con diferentes proporciones de Taiwan, Caña de Azucar y Melaza

    … PB fue el T1 (T99M1) con 4.08, menor pH el T10 (M33 C66) con 4.13, mayor TAD fue el T1 (T99M1) con 14.75 días y producción de CO2 fuel T7 (M95M5) con 43.06. En conclusión los tratamientos con diferentes proporciones de marango también demostra ron diferencias significativas con respectos a la …

    una Repository record for Estabilidad aerobica del ensilaje de marango con diferentes proporciones de Taiwan, Caña de Azucar y Melaza (opens in a new tab)

  13. Chemodynamical Properties of Simulated Late-type Galaxies

    … on the resulting chemistry of a new grid of M33-like disc simulations. The emphasis of the analysis is upon the resulting age-metallicity relations and metallicity distribution functions (in particular, the extreme metal-poor tail). Aspects of the work have been presented by Pilkington et al. …

    cent-lancashire Repository record for Chemodynamical Properties of Simulated Late-type Galaxies (opens in a new tab)

  14. Ecologie des stades larvaires et juvéniles du crabe tourteau (Cancer irrotatus Say, 11817), dans le détroit de Northumberland, Canada

    Le but de l’étude est de décrire les facteurs qui peuvent influencer le recrutement au fond du crabe tourteau, et de déterminer la relation entre la dynamique de population des larves et celle des juvéniles. Les aspects étudiés sont : l’abondance relative des différents stades larvaires, …

    moncton Repository record for Ecologie des stades larvaires et juvéniles du crabe tourteau (Cancer irrotatus Say, 11817), dans le détroit de Northumberland, Canada (opens in a new tab)

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